Browsing by Author "Molinari, S."

Now showing items 1-6 of 6

    • ATLASGAL – The APEX telescope large area survey of the galaxy at 870 μm 
      Schuller, F.; Menten, K. M.; Contreras, Y.; Wyrowski, F.; Schilke, P.; Bronfman Aguiló, Leonardo; Henning, Thomas; Walmsley, C. M.; Beuther, H.; Bontemps, S.; Cesaroni, R.; Deharveng, L.; Garay Brignardello, Guido; Herpin, F.; Lefloch, B.; Linz, H.; Mardones, D.; Minier, V.; Molinari, S.; Motte, F.; Nyman, L.-Å.; Reveret, V.; Risacher, C.; Russeil, D.; Schneider, N.; Testi, L.; Troost, T.; Vasyunina, T.; Wienen, M.; Zavagno, A.; Kovacs, A.; Kreysa, E.; Siringo, G.; Weiß, A. (ESO, 2009-02-20)
      Context. Thanks to its excellent 5100 m high site in Chajnantor, the Atacama Pathfinder Experiment (APEX) systematically explores the southern sky at submillimeter wavelengths, in both continuum and spectral line emission. ...
    • Distance of Hi-GAL sources 
      Mège, P.; Russeil, D.; Zavagno, A.; Elia, D.; Molinari, S.; Brunt, C. M.; Butora, R.; Cambresy, L.; Di Giorgio, A. M.; Fenouillet, T.; Fukui, Y.; Lambert, J. C.; Makai, Z.; Merello, Manuel; Meunier, J.C.; Molinaro, M.; Moreau, C.; Pezzuto, S.; Poulin, Y.; Schisano, E.; Schuller, F. (EDP Sciences S A, 2021)
      Aims. Distances are key to determining the physical properties of sources. In the Galaxy, large (>10 000) homogeneous samples of sources for which distance are available, covering the whole Galactic distance range, are ...
    • Molecular cloud catalogue from (CO)-C-13 (1-0) data of the Forgotten Quadrant Survey 
      Benedettini, M.; Traficante, A.; Olmi, L.; Pezzuto, S.; Baldeschi, A.; Molinari, S.; Elia, D.; Schisano, E.; Merello, M.; Fontani, F.; Rygl, K. L. J.; Brand, J.; Beltrán, M. T.; Cesaroni, R.; Liu, S. J.; Testi, L. (EDP Sciences, 2021)
      Context. New-generation spectroscopic surveys of the Milky Way plane have been revealing the structure of the interstellar medium, allowing the simultaneous study of dense structures from single star-forming objects or ...
    • The molecular environment of the Galactic star forming region G19.61–0.23 
      Santangelo, G.; Testi, L.; Leurini, S.; Walmsley, C. M.; Cesaroni, R.; Bronfman Aguiló, Leonardo; Carey, S.; Gregorini, L.; Menten, K. M.; Molinari, S.; Noriega Crespo, A.; Olmi, L.; Schuller, F. (ESO, 2010-06-03)
      Context. Although current facilities allow the study of Galactic star formation at high angular resolution, our current understanding of the high-mass star-formation process is still very poor. In particular, we still ...
    • SiO outflows in high-mass star forming regions: A potential chemical clock? 
      López Sepulcre, A.; Walmsley, C. M.; Cesaroni, R.; Codella, C.; Schuller, F.; Bronfman Aguiló, Leonardo; Carey, S. J.; Menten, K. M.; Molinari, S.; Noriega Crespo, A. (EDP SCIENCES, 2011-02)
      Context. Some theoretical models propose that O-B stars form via accretion, in a similar fashion to low-mass stars. Jet-driven molecular outflows play an important role in this scenario, and their study can help to understand ...
    • The SEDIGISM survey: First data release and overview of the galacti structure 
      Schuller, F.; Urquhart, J. S.; Csengeri, T.; Colombo, D.; Duarte Cabral, A.; Mattern, M.; Ginsburg, A.; Pettitt, A. R.; Wyrowski, F.; Anderson, L.; Azagra, F.; Barnes, P.; Beltran, M.; Beuther, H.; Billington, S.; Bronfman Aguilo, Leonardo Jaime; Cesaroni, R.; Dobbs, C.; Eden, D.; Lee, M. Y.; Medina, S. N. X.; Menten, K. M.; Moore, T.; Montenegro Montes, F. M.; Ragan, S.; Rigby, A.; Riener, M.; Russeil, D.; Schisano, E.; Sánchez Monge, A.; Traficante, A.; Zavagno, A.; Agurto, C.; Bontemps, S.; Finger, R.; Giannetti, A.; González, E.; Hernández, A. K.; Henning, T.; Kainulainen, J.; Kauffmann, J.; Leurini, S.; López, S.; Mac-Auliffe, F.; Mazumdar, P.; Molinari, S.; Motte, F.; Muller, E.; Nguyen Luong, Q.; Parra, R.; Pérez Beaupuits, J. P.; Schilke, P.; Schneider, N.; Suri, S.; Testi, L.; Torstensson, K.; Veena, V. S.; Venegas, P.; Wang, K.; Wienen, M. (Oxford University Press, 2021)
      The SEDIGISM (Structure, Excitation and Dynamics of the Inner Galactic InterstellarMedium) survey used the APEX telescope to map 84 deg2 of the Galactic plane between = −60◦ and +31◦ in several molecular transitions, ...